Ground-based coronagraphic observations of solar streamers

Details Ground-based coronagraphic observations of solar streamers Ground-based coronagraphic observations of solar streamers

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348...83a&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 83-86

Physics

Coronagraphs, Emission Spectra, Line Spectra, Solar Corpuscular Radiation, Space Observations (From Earth), Electron Density (Concentration), Soho Mission, Solar Corona, Solar Magnetic Field, Solar Physics

Scientific paper

A study which aims to demonstrate that ground based coronographs can observe coronal streamers and to give examples of the type of streamer properties that can be deduced from such observations is reported. Eclipse or balloonborne observations are not discussed. The emission line and white light (K coronagraph) observations relating to streamer electron density, magnetic field and polarization, population, intensity, large scale organization, rotation, temperature, and periodicities, are included. All known papers in this field are not reviewed but selected papers to demonstrate the types of work that can be done are used.

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